Infrared spectra and optical constants of astronomical ices: III. Propane, propylene, and propyne
RL Hudson, PA Gerakines, YY Yarnall, RT Coones - Icarus, 2021 - Elsevier
Infrared (IR) spectra of the hydrocarbon ices C 3 H 8 (propane), C 3 H 6 (propylene,
propene), and C 3 H 4 (propyne, methylacetylene) are relevant to the study of the low …
propene), and C 3 H 4 (propyne, methylacetylene) are relevant to the study of the low …
Chemical Evolution of CO2 Ices under Processing by Ionizing Radiation: Characterization of Nonobserved Species and Chemical Equilibrium Phase with the …
Astrophysical ices are being exposed to ionizing radiation in space environments, which
trigger new reactions and desorption processes. In the lab, such processing by radiation has …
trigger new reactions and desorption processes. In the lab, such processing by radiation has …
Characterization of acetonitrile ice irradiated by X-rays employing the procoda code – I. Effective rate constants and abundances at chemical equilibrium
GA Carvalho, S Pilling… - Monthly Notices of the …, 2022 - academic.oup.com
In this work, the chemical evolution of pure acetonitrile ice at 13 K irradiated with broad-band
soft X-rays (from 6 eV to 2 keV) is determined by using a computational methodology …
soft X-rays (from 6 eV to 2 keV) is determined by using a computational methodology …
Untangling the methane chemistry in interstellar and solar system ices toward ionizing radiation: a combined infrared and reflectron time-of-flight analysis
Pure methane (CH4/CD4) ices were exposed to three ionizing radiation sources at 5.5 K
under ultrahigh vacuum conditions to compare the complex hydrocarbon spectrum …
under ultrahigh vacuum conditions to compare the complex hydrocarbon spectrum …
Mapping the evolution of pure CO2 ices irradiated by ions, UV, and electrons using the upgraded PROCODA code (employing an effective rate constant ordering by …
Chemical reactions and desorption processes are being triggered by incoming ionizing
radiation over astrophysical ices in cold space environments. The quantification of these …
radiation over astrophysical ices in cold space environments. The quantification of these …
Chemical evolution of electron-bombarded crystalline water ices at different temperatures using the procoda code
S Pilling, CH da Silveira… - Monthly Notices of the …, 2023 - academic.oup.com
Water ices are a common component of cold space environments, including molecular and
protostellar clouds, and the frozen surfaces of moons, planets, and comets. When exposed …
protostellar clouds, and the frozen surfaces of moons, planets, and comets. When exposed …
Energetic processing of N2: CH4 ices employing X-Rays and swift ions: implications for icy bodies in the outer solar system
We experimentally address in this paper the physicochemical effects induced by ionizing
photons (energies from 6 to 2000 eV) and swift heavy ions (15.7 MeV 16 O 5+) in the icy …
photons (energies from 6 to 2000 eV) and swift heavy ions (15.7 MeV 16 O 5+) in the icy …
SO 3 formation from the X-ray photolysis of SO 2 astrophysical ice analogues: FTIR spectroscopy and thermodynamic investigations
V de Souza Bonfim, RB de Castilho… - Physical Chemistry …, 2017 - pubs.rsc.org
In this combined experimental–theoretical work we focus on the physical and chemical
changes induced by soft X-rays on sulfur dioxide (SO2) ice at a very low temperature, in an …
changes induced by soft X-rays on sulfur dioxide (SO2) ice at a very low temperature, in an …
Photochemistry and desorption induced by X-rays in water rich astrophysical ice analogs: implications for the moon Enceladus and other frozen space environments
Soft X-rays are an important agent for chemical processing in the Solar System and in the
interstellar medium. The photolysis and photodesorption processes of H2O-rich ices …
interstellar medium. The photolysis and photodesorption processes of H2O-rich ices …
Processing of N2O ice by fast ions: implications on nitrogen chemistry in cold astrophysical environments
Nitrous oxide, N2O, is found in the interstellar medium associated with dense molecular
clouds and its abundance is explained by active chemistry occurring on N2 rich ice surfaces …
clouds and its abundance is explained by active chemistry occurring on N2 rich ice surfaces …